The galaxy presents a relatively smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears roughly oblate in shape. The radial color gradient suggests a redder core transitioning to bluer outer regions. There's a subtle, slightly asymmetric extension visible that may indicate a minor tidal interaction or disruption.  The overall structure lacks distinct spiral arms or prominent dust lanes, appearing mostly spheroidal. The galaxy's light profile seems to fall off smoothly from the core, with no sharp cutoffs visible. The color distribution suggests an older stellar population dominating the central regions, while the outer areas may contain younger stars. Star formation appears relatively low. The object does not seem to be a strong merging candidate.