This galaxy exhibits a generally smooth, elliptical morphology. It appears moderately luminous, with a concentrated central bulge that gradually diffuses outwards. The color profile indicates a relatively older stellar population, with a noticeable shift towards redder hues in the outer regions of the galaxy, suggesting an absence of recent significant star formation. There is a subtle indication of a possible minor disturbance or interaction, based on a slight asymmetry in the galaxy's overall shape. No clear spiral arm structures or prominent dust lanes are visually apparent. Overall, the galaxy presents as a typical, well-evolved elliptical galaxy.
