The galaxy exhibits a generally smooth morphology, with a nearly round shape. There is no obvious presence of spiral arms or a distinct disk structure. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The color profile appears to be trending towards the redder end of the spectrum, suggesting a population of older stars and potentially lower levels of active star formation. There appears to be no significant signs of ongoing merging activity or tidal disturbances in the immediate vicinity of the galaxy. This appears to be a relatively massive system.
