The galaxy presents as a relatively compact object. There appears to be a dominant, centrally concentrated bulge component exhibiting a smooth, spheroidal morphology, with a slightly elongated appearance. The light distribution is relatively uniform across the bulge, suggesting an older stellar population and minimal ongoing star formation within this region.

There is evidence of at least one distinct feature close to the center. This feature has a noticeable color difference, with a redder hue compared to the central bulge region. This color may indicate a region of higher dust obscuration or a population of older, redder stars. There is also a possible faint extension or tidal tail visible. Given the observed features, this object is potentially undergoing or has recently undergone a minor interaction with another object.
