The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish in color, suggesting an older stellar population. Moving outwards from the bulge, the color transitions to a bluish hue, implying the presence of some younger, hotter stars in the outer regions. The overall shape is quite regular with no obvious spiral arms or bar structures visible. There's a subtle, almost imperceptible flattening, giving it a slightly oblate appearance. The light distribution is relatively symmetrical, and the edges of the galaxy appear diffuse, without sharp boundaries, indicating a gradual fading of stellar density into the intergalactic medium. There is no clear evidence of active galactic nuclei activity, major ongoing mergers, or prominent dust lanes within the observed image.
