The galaxy presents a generally smooth, elliptical morphology. A central, bright, concentrated bulge dominates the light profile, exhibiting a yellowish-orange hue, suggesting an older stellar population. A faint, extended disk component is present but ill-defined, with a subtle bluish tint on one side, possibly indicating a minor area of ongoing star formation, though this is not particularly prominent. There are no clear spiral arm structures or bar features discernible. Based on the redness of the bulge and faintness of the disk, there is a notable lack of significant recent or ongoing star formation activity across the galaxy as a whole. There is no evidence of any major mergers or tidal disturbances, though minor irregularities might be present. The galaxy is neither perfectly round nor highly elongated.
