The galaxy presents a generally smooth morphology, exhibiting a slightly elliptical shape. The light distribution is concentrated toward the center, suggesting a central bulge.  There is minimal evidence of spiral arm structure or distinct features; the galaxy appears largely featureless. The color profile indicates a redder hue overall, particularly in the core, which could suggest an older stellar population and lower levels of ongoing star formation. The outer regions show a slight bluer tint in the green/blue wavelengths suggesting more recent pockets of star formation, although the overall star formation rate appears subdued. There is no apparent disruption indicating recent major mergers.
