The galaxy appears as a relatively smooth, elliptical object with a concentrated central bulge. The light distribution is somewhat spheroidal, with a gradual decline in brightness moving outward from the core. There's a subtle color gradient present, with a slightly redder hue towards the central region and a bluer tint in the outer parts of the galaxy. No distinct spiral arm structures or prominent dust lanes are apparent in the image. The galaxy exhibits a generally uniform texture, suggesting an older stellar population. There are no signs of ongoing major mergers, although there is some slight disturbance in the galaxy's symmetry. The galaxy does not appear to be actively forming stars at a high rate, exhibiting low specific star formation.
