The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The light distribution appears to be dominated by an extended, spheroidal bulge component. The color gradient is subtle, trending from a slightly bluer hue in the outer regions to a more yellowish/reddish hue toward the core, suggesting a stellar population that is older and/or more metal-rich toward the galaxy's center. There is little evidence of spiral arm structure or significant dust lanes. A very faint disk may be present, but it is not prominent. There are no obvious signs of ongoing major mergers or tidal disturbances, though subtle asymmetries may indicate minor interactions.
