The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. There's a noticeable color gradient, shifting from a yellow-white core to a more subdued, slightly bluer hue in the outer regions. The core appears quite luminous, suggesting a high stellar density. The outer edges of the galaxy show hints of a fainter disk component, though the image resolution limits detailed analysis of any spiral arm structures. There is little indication of recent or ongoing major merger activity, though a minor disturbance cannot be ruled out given the low-resolution imaging. The overall morphology points towards a relatively evolved galaxy with a dominant older stellar population.
