The galaxy presents as a single, relatively smooth object with a concentrated central bulge. There is a noticeable radial color gradient, with a yellowish-white core transitioning to a bluer halo at the outer edges. The apparent ellipticity is low, suggesting a nearly circular morphology. There are no obvious spiral arms or distinct dust lanes visible. There is no evidence of tidal tails or other significant morphological distortions indicative of recent merger activity. The galaxy's color profile implies the presence of an older stellar population dominating the central bulge, with potentially younger, bluer stars contributing to the outer halo regions.
