The galaxy appears as a relatively smooth, elliptical-like structure. Its light profile suggests a concentrated central region that gradually fades outwards. The color is predominantly yellow, hinting at a population of older stars, with some regions appearing more reddish. This colour profile suggests ongoing star formation activity. The galaxy appears quite compact, lacking any prominent spiral arms or distinct morphological features. There is no obvious dust lane or significant sign of tidal interactions. A possible faint distortion on one side might suggest a recent minor merger or gravitational interaction. Overall, the morphology indicates a fairly evolved galaxy with a likely substantial stellar mass.