The galaxy presents as a single, relatively smooth object with a concentrated central bulge. It appears elliptical in shape, exhibiting a high degree of roundness. Coloration is primarily yellow-orange, indicating a population of older stars. There is no discernable spiral structure or prominent dust lanes. Minimal signs of ongoing star formation are apparent from the color profile. The galaxy appears to be relatively isolated, showing no significant tidal distortions or indications of major mergers. There is a slight hint of a possible minor disturbance or a faint, unresolved companion.
