The galaxy exhibits a predominantly smooth morphology, with a possible, albeit faint, disk-like structure. It appears elongated, displaying a cigar-like shape. The galaxy's core appears centrally concentrated, surrounded by a fainter halo. There is no indication of ongoing major merging events. Faint, small features suggest that it could have minor disturbances. Star formation appears to be present, at a low rate. Overall, the galaxy's stellar population appears relatively old.