The galaxy presents as a somewhat elliptical object with a smooth, diffuse light distribution. The central region appears brighter and has a yellowish hue, suggesting a concentration of older stellar populations. Moving outward from the center, the color gradually shifts to a slightly bluer tone in the outer regions. The light distribution is quite even, with no clear indications of spiral arms or strong dust lanes. The galaxy appears to be relatively isolated, with no obvious signs of ongoing tidal interactions or merging events. Its shape is more elongated than circular, with a ratio of major to minor axes indicating a mild degree of flattening. There is no clear indication of a distinct nucleus within the bright central bulge.
