This galaxy appears to be a relatively smooth, elliptical galaxy with a slight elongation. There is a bright central bulge that gradually fades out into a diffuse halo. The light distribution suggests an older stellar population, with a dominant yellow-red hue indicating a lack of significant ongoing star formation. There are no obvious spiral arms or dust lanes visible. The overall structure seems largely undisturbed, suggesting it has not undergone a recent major merger. Minor disturbances cannot be ruled out, but are not readily visible. The color is slightly bluer in the center, which is a sign of a lower age of the stars that form it.
