The galaxy presents as an elliptical or lenticular structure. It appears elongated, with a cigar-like shape. The galaxy exhibits a generally smooth texture with no apparent spiral arm structures or significant dust lanes visible. The central region is characterized by a bright, concentrated luminosity that fades towards the edges of the galaxy. The color profile suggests an older stellar population, as indicated by the redder hue, implying lower recent star formation activity. There is no obvious evidence of ongoing major merger events or significant tidal disturbances in its immediate vicinity, although minor disturbances cannot be ruled out.
