The galaxy presents a smooth, elliptical morphology with an elongated shape. The central bulge exhibits a concentrated luminosity gradient, suggesting a high stellar density. The color profile is generally consistent with an older stellar population, with a noticeable shift towards redder hues compared to bluer star-forming regions. There's no indication of prominent spiral arm structures or significant dust lanes. Subtle irregularities in the outer regions may suggest past minor interactions, but overall the galaxy appears relatively undisturbed.
