The galaxy presents as a generally smooth object. It appears to be elliptical in shape, with the ratio of the major to minor axis close to 1. The galaxy exhibits a central concentration of light, with luminosity gradually decreasing towards the outer edges, suggestive of a bulge. The light from the bulge has a yellowish hue, and is likely dominated by older stellar populations. The galaxy does not show any clear evidence of spiral arms, a prominent disk, or ongoing major mergers. There are no signs of significant star formation activity in the outer parts.
