The galaxy presents a generally smooth appearance, with a dominant central bulge. The overall shape appears close to round, though there are slight deviations suggesting it is not perfectly spherical. There is faint evidence of a potential disk or featured structure, but it is not prominent. The color of the bulge is a yellow-orange hue, suggestive of an older stellar population. There is an indication of some minor disturbance or potential merging activity, characterized by a faint, irregular feature that is redder in color. Overall, the galaxy appears to be in a relatively quiescent state, showing evidence of past interactions.
