The galaxy appears to be a relatively smooth, elliptical galaxy with a noticeable central bulge. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a moderately elongated shape, with the major axis oriented in a northeast-southwest direction. There is a color gradient, with the core of the galaxy appearing whiter and the outer regions trending towards a more yellow/red hue. This could indicate an older stellar population dominating the outer regions. The galaxy appears to be relatively isolated, showing no major signs of tidal disturbances or ongoing mergers with other galaxies. There is a slight asymmetry in the distribution of light within the galaxy, with a somewhat brighter region on one side of the core compared to the other.
