The galaxy presents as a slightly elongated, cigar-shaped structure with a relatively smooth overall appearance. It exhibits a concentration of luminosity towards the central region, suggesting a prominent galactic nucleus or bulge. The light distribution appears to diminish gradually outwards from the center. There are subtle indications of possible minor disturbances in its structure, or potentially faint spiral arm features that are tightly wound. The galaxy appears primarily yellow-reddish in color, indicating an older stellar population with lower levels of star formation. It does not appear to be undergoing a major merger or strong tidal interaction.
