The galaxy presents as a centrally concentrated object with a generally smooth appearance. It displays an elliptical or lenticular morphology, with an approximate effective radius of several kiloparsecs. The light profile exhibits a radial gradient, with a brighter core gradually diminishing outwards. The color distribution suggests the presence of an older stellar population, contributing to its reddish-yellow hue. There is no strong evidence of significant spiral arm structure, prominent dust lanes, or ongoing major merger activity. However, there are hints of minor irregularities in the outer regions, possibly indicative of past or ongoing minor interactions. Overall, the galaxy is characterized by its relatively quiescent nature and the dominance of evolved stellar populations.
