The galaxy presents as a relatively smooth, but not perfectly spherical, structure. There is a slight elongation apparent. The color profile suggests a moderate degree of star formation. A central concentration of older stars contributes to the overall luminosity. There is evidence of disturbed morphology, possibly indicating a past or ongoing interaction, as subtle tidal features may be present. The observed color profile implies a range of stellar populations, with regions of ongoing star formation intermixed with areas dominated by older, redder stars. The galaxy's overall appearance suggests a system that may be transitioning in its evolutionary state, exhibiting characteristics of both elliptical and spiral galaxy types.
