The galaxy presents a largely smooth morphology, appearing elliptical or lenticular. A central bulge is readily apparent, exhibiting a concentrated brightness that gradually fades into the outer regions. The color profile suggests a population of older stars, likely with a lower rate of ongoing star formation, contributing to its reddish hue. There's a general lack of distinct spiral arm structures or prominent dust lanes, further supporting the classification as an early-type galaxy. The overall shape leans towards spherical, showing only a slight deviation towards an elongated form. Faint signs of possible tidal disturbances indicate a history of interactions or mergers, though currently, the galaxy appears largely undisturbed.
