The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth, featureless morphology. Its light profile suggests a high degree of central concentration, with brightness decreasing gradually towards the outer regions. A slight elongation is observed, indicating a deviation from a perfect circular shape. The color appears generally homogenous across the galaxy, indicative of an older stellar population with minimal ongoing star formation. No distinct spiral arms, dust lanes, or prominent HII regions are visible. There are no obvious signs of recent or ongoing merger activity, such as tidal tails or disrupted morphology, and no central bar is visible.
