The galaxy appears as a relatively smooth, elliptical structure with a noticeable central bulge. The color profile suggests an older stellar population, primarily exhibiting redder hues concentrated towards the core, with a slight shift towards green in the outer regions. The overall shape is somewhat elongated, though not extremely so, with the long axis showing a degree of internal complexity in luminosity distribution. There are no prominent spiral arms or distinct dust lanes visible. The galaxy's morphology is consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy, displaying no major disturbances or signs of ongoing merging activity.
