The galaxy presents a mostly smooth morphology, with a central bulge region exhibiting a concentrated, yellowish hue, possibly indicative of an older stellar population. A faint, diffuse disk is observed surrounding the bulge. The disk appears relatively featureless, though there is a hint of a spiral arm structure along the lower edge of the galaxy, appearing as a minor disruption from the overall smoothness. The shape appears moderately elliptical, deviating from a perfectly circular form, suggesting it is an intermediately-inclined disk galaxy. No signs of ongoing major mergers or significant tidal disturbances are readily apparent. The overall structure suggests a galaxy that is nearing the end of active star formation, with a dominance of older stellar populations.
