The galaxy presents as a relatively smooth, elongated structure, suggestive of an elliptical morphology or possibly a highly inclined spiral. The central region exhibits a pronounced brightness, indicating a concentration of stellar mass. The outer regions gradually fade into the background, with no distinct spiral arms or prominent features immediately discernible. There appears to be a mild asymmetry in the light distribution. The color profile is reddish, implying an older stellar population and reduced ongoing star formation. The overall light distribution is well-fit by a Sersic profile, indicating a centrally concentrated and relatively smooth structure. There may be some merging or tidal interactions taking place, but these are minor. The absence of significant blue light suggests that active star formation is limited in this galaxy.
