The galaxy exhibits a generally elliptical morphology, appearing elongated along a defined major axis. The light distribution suggests a relatively smooth profile, with a concentrated central bulge. The core displays a yellowish hue indicative of an older stellar population. The outer regions of the galaxy show a subtle shift towards a bluer color, potentially reflecting areas of more recent, though diminished, star formation. There is no strong evidence of spiral arm structure. Minor irregularities may be present in the outer regions. The overall appearance suggests a galaxy that is somewhat evolved, with star formation occurring at a low rate.
