The galaxy presents an elliptical morphology, appearing largely smooth and somewhat elongated in shape. Its core exhibits a concentrated, luminous region, likely indicating a substantial stellar population and/or active galactic nucleus. A diffuse, more extended halo surrounds the central region, with the light gradually fading away from the core. There are some faint irregular features, possibly minor tidal disturbances or remnants of past interactions, but these do not significantly disrupt the overall smooth elliptical profile. The galaxy exhibits a reddish hue, consistent with an older stellar population and potentially a lower star formation rate.
