The galaxy presents as an elliptical or lenticular morphology, elongated along one axis, indicative of a flattened spheroidal shape. The central region exhibits a concentrated, bright yellowish-white core, suggesting a substantial population of older stars or potentially an active galactic nucleus. Progressing outwards from the core, the light gradually diminishes. The presence of a faint blueish hue on the outer edges indicates the presence of some young stars undergoing active formation. The overall color profile suggests a mix of stellar populations, with older, redder stars dominating the core and younger, bluer stars contributing to the outer regions. There is no apparent dust lane or spiral arm structure discernable in the image, which supports the classification as an elliptical or lenticular galaxy. The smooth appearance suggests a lack of recent major mergers. Faint disturbances cannot be ruled out.