The object presents as a centrally concentrated, relatively smooth galaxy. The light profile appears fairly uniform with a slight radial gradient, indicating a higher concentration of luminous material towards the core. There is very little evidence of distinct spiral arm structures or prominent dust lanes. The overall shape appears approximately circular, with a high degree of central symmetry. There is a possible subtle asymmetry in the outer isophotes suggesting a minor gravitational interaction. No prominent tidal tails or bridges are visible. The galaxy exhibits a yellow-white color, suggesting an older stellar population. The galaxy appears to be relatively undisturbed, and likely has not undergone a major merger in the recent past.