The galaxy presents a largely smooth morphology, with a concentrated central bulge. The overall shape appears somewhat elliptical, tending toward being in between round and elongated with no obvious spiral arm structure. The color profile indicates an older stellar population, with a yellowish-orange hue dominating the central region, suggesting a higher concentration of evolved stars. A faint blue-ish tinge is observed in the outer regions, potentially indicating some low-level ongoing star formation, but this is not a dominant feature. There is no obvious evidence of major mergers or significant tidal disturbances. Any perturbations seem minor if they exist at all.
