The galaxy exhibits a generally smooth morphology, with a slight elongation suggesting a possible transition between elliptical and lenticular. The central region displays a bright, concentrated bulge. There is very little visible structure in the galaxy image, with no apparent spiral arm or bar features. There may be a faint, diffuse halo surrounding the central region. The color profile indicates an older stellar population, with a reddish hue dominating the galaxy. The relative smoothness, absence of prominent disk features, and the reddish color suggest a relatively low star formation rate. There seems to be a slight distortion in the top region of the galaxy, indicating a possible small disturbance in the surrounding area, or a minor merger that does not disrupt the main body of the galaxy.
