The galaxy appears as a single, relatively smooth, spheroidal object. It exhibits a concentrated light profile with a bright central region that gradually fades outwards. The galaxy presents a moderate red hue, suggesting a population of older stars and a lower rate of active star formation. There may be a slight visual indication of a possible interaction or minor disturbance within the galaxy's structure, however, it seems generally undisturbed. The galaxy appears to be roughly circular. No distinct spiral arms or a prominent disk component are visible in the image.
