The observed galaxy presents as a relatively smooth, elongated structure. The primary body of the galaxy exhibits a concentrated central region, possibly indicative of a galactic bulge. The color profile suggests a population of older stars, as evidenced by the reddish hue concentrated towards the central regions, with a bluer component towards the outer edges, likely indicating ongoing, albeit limited, star formation. The galaxy displays a general lack of prominent spiral arm structures or significant dust lanes, hinting towards a classification as a lenticular or possibly an elliptical galaxy, depending on the degree of three-dimensional ellipticity. No apparent major tidal disturbances or indications of ongoing merging activity are visible in the immediate vicinity. The estimated size suggests that we are observing a galaxy that is approximately 6.8 kpc across.
