The galaxy presents as a predominantly smooth, elliptical structure with a concentrated central bulge exhibiting a bright yellowish hue. There is little evidence of spiral arms or significant dust lanes. The overall shape is highly rounded. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger or strong tidal distortions. A subtle, reddish elongation is apparent on one side, suggesting a potential minor disturbance or interaction, possibly a smaller companion galaxy. The galaxy's color index suggests a population of older stars and a relatively low rate of current star formation.
