The galaxy presents as a somewhat smooth and diffuse object, elongated in shape, appearing slightly cigar-shaped rather than perfectly round. There is a subtle central concentration of light, suggesting a possible bulge component, though it is not sharply defined. Faint, diffuse extensions emanate from the central region. The galaxy exhibits a general yellowish color, which might indicate an older stellar population and a relatively low rate of ongoing star formation. There are no prominent spiral arms, dust lanes, or other easily discernible features, implying a structure dominated by older stars. Some minor disturbances, such as small extensions, are present in its morphology. The system appears to be a relatively isolated galaxy and is not currently undergoing any major mergers.
