The galaxy presents a generally smooth, elliptical morphology. The light profile exhibits a concentrated central bulge that is yellowish in color, suggestive of an older stellar population. Fainter, bluish light extends outwards from the bulge, possibly indicating some recent star formation, although not at a high rate. The galaxy is elongated, appearing as a flattened spheroid, rather than a perfectly circular object. No distinct spiral arm structures or prominent dust lanes are discernible. There is a very slight asymmetry to the outer edges of the galaxy, potentially indicative of a past minor interaction or disturbance.
