This galaxy appears to be undergoing a merger or tidal interaction. The primary body of the galaxy exhibits an irregular morphology, lacking a well-defined spiral or elliptical structure. There is a distinct, although somewhat diffuse, secondary object in close proximity to the main body, indicating a possible companion galaxy or tidal debris. The central region of the galaxy is brighter and has a yellow/orange color, which may indicate an older stellar population, while bluer hues are seen within what appear to be disrupted structures. Given the disturbed morphology and the evidence of interaction, star formation may be elevated in localized regions due to gas compression from the gravitational interaction. The absence of a prominent disk suggests the galaxy is either an elliptical galaxy caught in an interaction, or a spiral galaxy that has been significantly disrupted. Further spectral analysis would be required to determine the age of the stellar populations and the star formation rate more precisely, but the visual appearance indicates a dynamically active system.
