The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light profile appears diffuse, lacking distinct spiral arms or prominent dust lanes. The color index suggests a population of older stars. There's a slight elongation, indicating it is closer to "in between" on the round to cigar-shaped scale. Based on the lack of strong distortions or tidal features, there's no clear evidence of a recent major merger. The galaxy appears to be mostly undisturbed.