This galaxy exhibits a generally smooth morphology, appearing elliptical in shape. The central region is dominated by a bright, concentrated core, suggesting a high density of stars. There's a noticeable color gradient, with the core displaying a bluer hue, possibly indicative of a younger stellar population or ongoing star formation, and the outer regions appearing redder. The lack of distinct spiral arms or a well-defined disk suggests a classification towards the elliptical end of the Hubble sequence. There are slight irregularities in the outer regions, but not significant enough to classify it as a merging system. Overall, this galaxy seems to be a fairly evolved system, potentially with a more recent burst of star formation in its central regions.
