The galaxy presents as a somewhat elongated, elliptical structure. It exhibits a smooth, centralized concentration of light, suggesting a dominant bulge component. The color profile appears generally reddish-yellow, potentially indicative of an older stellar population and/or significant dust obscuration. There is little evidence of distinct spiral arms or active star-forming regions based on its overall smooth appearance. Its shape is decidedly cigar shaped, more oblong than spherical. There are no visible signs of any major merging activity or tidal disturbances. Overall, this appears to be a relatively passive, early-type galaxy at a moderate redshift.
