The galaxy presents a generally smooth morphology, suggesting a relatively evolved system. It appears elongated, exhibiting a cigar-like shape, with the ratio of the major to minor axis being fairly substantial. The light distribution appears centrally concentrated but extended, with no distinct spiral arm structures visible. There is a slight color gradient across the galaxy, with the central regions potentially appearing redder compared to the outer edges, which appear slightly bluer, indicating ongoing, but relatively low, star formation. The galaxy appears relatively isolated with no obvious signs of ongoing major mergers or strong tidal interactions with other galaxies. There may be some indication of a minor disturbance, but nothing dramatic. 
