The galaxy appears as a generally smooth, elliptical structure, exhibiting a concentrated central bulge that fades gradually into the outer regions. The light distribution is relatively uniform, lacking distinct spiral arms or prominent dust lanes. The galaxy’s color profile shows a dominant reddish-yellow hue, indicating a population of older stars and a relatively low rate of current star formation. It appears largely undisturbed, without significant tidal tails or signs of a major ongoing merger. Subtle asymmetries may be present upon closer inspection, suggesting minor disturbances or past interactions, although the overall morphology remains largely undisturbed.
