The galaxy presents a generally smooth and rounded morphology. Its color profile appears primarily red-shifted, suggestive of an older stellar population. There is very little evidence of spiral arm structure or significant dust lanes. The central bulge region seems quite prominent, with the overall light profile gently decreasing in intensity moving outwards from the center. The galaxy appears relatively isolated with no apparent signs of ongoing major mergers or tidal disturbances. Faint extensions of the outer halo are visible, though they are ill-defined and blend into the background sky noise. Overall, this galaxy exhibits characteristics of a quiescent elliptical galaxy with minimal ongoing star formation.
