The galaxy presents as an elongated, cigar-shaped structure. The light distribution is relatively smooth and centrally concentrated, with a gradual decrease in intensity moving outwards from the core. The primary color is a yellowish-orange, suggestive of an older stellar population dominated by redder stars. There is minimal evidence of distinct spiral arms or active star-forming regions. The galaxy lacks a prominent disk component and appears generally featureless. Any disturbances are minor and do not disrupt the overall smooth morphology of the galaxy.
