The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge that appears slightly elongated. The color gradient suggests a stellar population dominated by older, redder stars within the core, with a gradual shift towards bluer hues in the outer regions, possibly indicating more recent star formation. There appears to be a slight asymmetry in the galaxy's light distribution, with a subtle extension of the halo on one side. No prominent dust lanes or spiral arm structures are clearly discernible. There may be a minor tidal disturbance, though difficult to ascertain from the image alone. Overall, it is a relatively compact galaxy, with an estimated effective radius on the order of one kiloparsec.
