The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, which appears approximately circular and dominates the overall luminosity. The color profile shows a yellowish-orange hue, suggestive of an older stellar population, potentially indicating a lower rate of current star formation. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. A slight asymmetry in the outer regions may suggest minor tidal interactions or past merger events, but the overall structure is largely undisturbed. The galaxy appears to be relatively isolated, with no immediate, gravitationally interacting companions visible in the immediate vicinity.
