The galaxy exhibits a morphology leaning towards a smooth appearance, yet displaying certain features suggestive of a disk-like structure. The shape is somewhat rounded, with a subtle elongation detected. There is no strong indication of a major merger event, though minor disturbances cannot be entirely ruled out.

The galaxy displays a moderate amount of recent or ongoing star formation. The optical colors suggest a population of intermediate-age stars, contributing to its observed luminosity. Given the estimated size, the galaxy appears relatively compact.
