The galaxy presents a primarily smooth morphology, suggesting a relatively old stellar population. It exhibits a centrally concentrated bulge with a somewhat elliptical shape. A faint disk component is suspected, displaying bluer colors indicative of ongoing, but relatively low, star formation. There may be signs of minor disturbances in the galaxy's structure, potentially caused by a past or ongoing minor merger event, or tidal interaction. The object's profile is more in-between than cigar-shaped or fully round. The color gradient transitions from a yellowish core to bluer hues in the outer regions.
