This galaxy presents as a relatively bright, elliptical or lenticular system with a noticeable reddish hue, indicative of an older stellar population. The galaxy's shape is somewhat elongated, appearing more cigar-shaped than perfectly spherical. The light distribution seems smooth, showing no prominent spiral arms or distinct features typically associated with actively star-forming regions. There's a subtle central concentration of light, potentially indicating a bulge or a small active galactic nucleus, though its intensity seems moderate. There are indications of minor disturbances to the morphology, suggestive of possible past interactions or mergers. The overall structure appears relatively undisturbed, with no clear signs of ongoing major merging activity. The estimated size suggests a moderately large galaxy.
