The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. A distinct nucleus is not readily apparent, with the light gradually decreasing outwards from the core. The overall color appears somewhat reddish-yellow, suggesting a population of older stars, particularly in the central region, with relatively low ongoing star formation activity. There is a very subtle hint of bluer colors in the outskirts, possibly indicative of a younger stellar population there, but this could also be image noise. No obvious spiral arms, bars, or significant dust lanes are visible. There are no signs of any major tidal disturbances, merging events, or other significant morphological irregularities. The galaxy appears relatively isolated.
