The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its color profile suggests a dominant population of older stars in the core, indicated by the yellowish-orange hue, surrounded by a faint, greenish-blue halo. The lack of distinct spiral arm structures or prominent dust lanes points towards an elliptical classification or a late-stage spiral galaxy with a well-developed bulge. There are no obvious signs of ongoing major mergers or tidal disturbances in this image, implying relative isolation or a state of dynamical equilibrium. The relatively homogenous color distribution further suggests a lack of significant star formation. The overall roundness of the galaxy indicates a relatively high degree of rotational symmetry.
