The galaxy presents a generally smooth morphology, likely a lenticular or elliptical type given the lack of prominent spiral arms or a well-defined disk. There is some evidence of a slight flattening of the light distribution, but the overall shape is fairly spheroidal. The central region displays a concentrated luminosity, suggesting a substantial stellar population in the core. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in the outer regions to a redder color toward the center. This potentially indicates a population of younger, bluer stars in the outer regions and older, redder stars dominating the core. There are hints of slight disturbances in the galaxy's structure, which may be the result of a past minor merger event or internal dynamics. The overall structure suggests a relatively evolved galaxy with moderate star formation activity.
