The galaxy presents a generally smooth appearance, exhibiting a concentrated central bulge of moderate intensity. Its overall shape appears somewhat elliptical, though tending more towards an intermediate, rather than a completely spherical, form. There is no clear evidence of a spiral disk or spiral arms. The light profile appears to be largely smooth, with no strong knots of star formation or prominent dust lanes visible in the image. Based on the subtle asymmetry, and nearby object, it may be weakly interacting with another galaxy, but it is likely not a major merger event. The color suggests a mix of stellar populations, though there is a slight dominance of older stars, which may lead to less current star formation.
