The galaxy appears to be an elliptical type. It has a smooth, centrally concentrated light distribution. The light tapers off gradually from the core, indicating a lack of distinct spiral arms or a well-defined disk structure. It appears moderately bright with a slight elongation, deviating somewhat from a perfectly circular shape. No obvious dust lanes or signs of active star formation regions are readily apparent in this image. The galaxy appears relatively isolated, without any close companions or significant tidal distortions, which suggests it is not currently undergoing a major merging event, though there is a slight irregular shape.