The galaxy presents as a slightly elongated, diffuse object with a noticeable central bulge. The color profile suggests a relatively even mix of stellar populations across the galaxy, although the central region appears to exhibit a somewhat greener hue, potentially indicative of ongoing star formation activity. There is no clear spiral arm structure visible; instead, the galaxy presents a smoother, more amorphous appearance. Faint tidal features, possibly indicative of a past or ongoing merger event, cannot be ruled out. Overall, the galaxy appears to be in an intermediate stage of morphological evolution, exhibiting characteristics of both elliptical and spiral galaxies. Further spectroscopic analysis would be valuable to ascertain the precise star formation rate and redshift.
