Observed galaxy exhibits an overall elliptical morphology with a relatively smooth light distribution. The central region appears to be dominated by an older stellar population, indicated by its yellowish-red hue and a high concentration of light. The outer regions show a bluer tint, suggesting the presence of a younger stellar population and potentially ongoing star formation. There are hints of a faint disk-like structure, but no distinct spiral arms are visible. The galaxy's shape is slightly elongated, but not significantly cigar-shaped. There may be signs of minor disturbances or interactions. Overall, the galaxy appears to be a fairly massive system with moderate star formation activity.
