The galaxy appears to be a lenticular or possibly a spiral galaxy, observed at an oblique angle. It exhibits a flattened, elongated shape, resembling a cigar. The central bulge is prominent, appearing smooth and concentrated. A faint, disk-like structure can be discerned, although details such as spiral arms are not clearly defined. There is a general lack of distinct features, giving it a relatively uniform appearance. The galaxy's color is generally consistent, with a slightly yellowish hue, implying an older stellar population. There is no evidence of ongoing major mergers, although a subtle asymmetry may suggest a minor interaction or disturbance in the past.
