The galaxy presents as a fairly round, smooth object with a concentrated central bulge. Its overall color profile leans towards the redder end of the spectrum, indicative of an older stellar population and reduced star formation activity. There appears to be a subtle color gradient, with the core exhibiting a slightly more yellow hue compared to the outer regions. No distinct spiral arms or bar structures are discernible. The galaxy’s morphology suggests a classification as an elliptical galaxy, possibly an early-type spiral galaxy. The high degree of smoothness indicates that major mergers are unlikely, and a relatively undisturbed evolutionary history is probable.
