The galaxy presents an elliptical morphology, with an overall smooth appearance. The galaxy displays a central concentration of light, gradually fading towards its outer edges.  The color profile appears generally redder at the core, suggesting a higher concentration of older stars.  Moving outwards, the galaxy exhibits some bluer patches in the periphery, possibly indicating regions of more recent or ongoing star formation.  There is no obvious spiral arm structure visible, and the shape is more akin to a flattened spheroid.  There's evidence of some morphological disturbance or interaction, a slight asymmetry in the overall shape.  This disturbance may manifest as a faint tidal feature or the result of a minor merger event. The galaxy's estimated size suggests it is a moderately large system.
