The galaxy exhibits a complex morphology, possibly resulting from an ongoing or recent merger event. The primary component appears to be a relatively smooth, somewhat elliptical structure with a concentrated central region. The color of this component is predominantly red/yellow, suggesting a population of older stars and lower rates of star formation.

A secondary, bluer component is observed in close proximity to the primary one. This bluer region indicates the presence of younger, hotter stars and potential star-forming activity. There are indications of tidal features or faint extensions emanating from the galaxy, particularly around the bluer component, supporting the hypothesis of gravitational interaction or tidal disruption. The overall shape is irregular, with the two distinct components not smoothly integrated, further suggesting a disturbed system. Further investigation, including spectroscopic analysis, would be beneficial to determine the redshifts of each component and confirm the merger hypothesis.
