The galaxy presents as a centrally concentrated, smooth structure with a generally elliptical morphology. The light distribution appears relatively uniform across the main body of the galaxy, with no apparent distinct features such as spiral arms or a prominent bar. There is a slight elongation present, giving it an intermediate roundness classification. The galaxy's color suggests an older stellar population, with a relatively redder hue compared to bluer, star-forming galaxies. Evidence of minor disturbances is present in the galaxy's structure; a possible ongoing or recent minor merger is contributing to this. There is a distinct lack of major merger characteristics. The galaxy's overall appearance indicates that star formation is relatively low compared to its overall stellar mass.
