The galaxy presents a concentrated, bright central bulge with a yellowish hue, suggesting an older stellar population. Fainter and bluer light surrounds the center, with possible hints of spiral arm structure emerging from the core region, though not clearly defined. The disk appears relatively smooth and lacks prominent dust lanes or distinct star-forming regions. There are no obvious signs of a major merger event, such as tidal tails or highly distorted morphology, but there are slight indications of irregularities in the outer regions of the disk, suggesting a possible minor interaction. The galaxy possesses an estimated size of approximately 19 arcseconds in diameter. Overall the galaxy appears to have characteristics of both elliptical and spiral galaxies. 
