The galaxy presents as a diffuse, moderately luminous object with a noticeable, though not entirely smooth, structure. There appears to be a central concentration of light, suggestive of a galactic bulge. The overall shape is generally elliptical, exhibiting some degree of roundness, however there are features disrupting the even light distribution. There is a suggestion of an ongoing or recent minor interaction or disturbance impacting the structure. The color profile indicates a population of older stars, contributing to the observed redder hue. The galaxy is likely a moderately massive system with a modest rate of star formation, though the presence of bluer regions within the larger structure hints at possible younger stellar populations scattered throughout the galaxy. There is a noticeable absence of spiral arm structure. Overall, the galaxy is a slightly disturbed early-type galaxy undergoing mild evolutionary processes.
