The galaxy presents as a relatively compact object with a bright, concentrated core. The overall morphology suggests a system that is primarily smooth in appearance. The light distribution appears centrally concentrated, fading outwards. There is a slight elongation. The color profile indicates a population of stars with a mix of ages, with the core exhibiting a bluer hue and the outer regions trending towards redder tones, suggesting either ongoing star formation in the core or a younger stellar population. There appears to be no distinct spiral arm structure or bar feature discernable in the image. Overall, the system appears relatively undisturbed, showing no obvious signs of a major merger event, with only slight asymmetries that might indicate a minor interaction in its past or present.
