The galaxy presents an overall elliptical morphology, appearing more rounded than elongated. The light distribution suggests a relatively smooth profile, with a central concentration that diffuses outwards. A slight asymmetry is visible, potentially indicating a minor disturbance or interaction.

The galaxy's color profile suggests an older stellar population, leaning towards a redder hue in the outer regions. A central area has a slightly bluer tint. There is visual evidence suggesting a possible minor merger or tidal interaction. Overall, this appears to be a galaxy undergoing complex gravitational interactions or a recent merger event.
