The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity extending outwards. The overall shape is elongated, presenting a cigar-like appearance. The core of the galaxy has a yellow-white hue suggesting an older stellar population. Subtle blueish colorations can be observed in the outer regions of the galaxy, potentially indicating some ongoing or recent star formation activity, although this is not pronounced. No significant signs of spiral arms, dust lanes, or tidal disturbances are visible. There are no other merging galaxies nearby or signs of any interactions with the surrounding galactic environment.
