The galaxy presents as a moderately luminous object with a generally elliptical morphology. It displays a smooth, concentrated central bulge that graduates into a fainter, more diffuse halo. The color profile suggests an older stellar population, with a notable presence of redder hues dominating the core. Some bluer colors can be seen surrounding the core. There appears to be no distinct spiral structure or significant dust lanes visible in this image. Minor disturbances in the outer regions hint at a possible past or ongoing interaction, but the overall structure remains largely undisturbed. The galaxy does not appear to be undergoing a major merging event.
