The galaxy presents as a moderately luminous, elongated structure. It is characterized by a smooth, diffuse light distribution, suggesting a lack of prominent spiral arms or significant dust lanes. The central region exhibits a slightly higher surface brightness than the outer regions. The overall color appears to be on the redder side, which is indicative of a relatively older stellar population and lower ongoing star formation. There may be some minor disturbances within the disk, but it is unlikely this galaxy is undergoing any sort of major disturbance or merger. The shape appears cigar-like, with a width close to half the size of its length. Overall, the galaxy morphology aligns with that of an elliptical or lenticular type.
