The galaxy presents as a relatively smooth, rounded object with a concentrated central bulge. There is little evidence of spiral arm structure or prominent dust lanes. The core exhibits a yellowish hue, potentially indicative of an older stellar population, while the outer regions appear slightly bluer. Overall, the galaxy appears quiescent, with no obvious signs of active star formation. A slight elongation is detectable, suggesting that the galaxy is not perfectly spherical, but rather somewhat elliptical in shape. There is no indication of ongoing major mergers or tidal disturbances.
