The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a well-defined central bulge that appears bright and concentrated. The galaxy displays an overall oblong shape, with the light distribution gradually fading towards the outer edges. The color profile suggests a population of older stars, as indicated by the presence of redder hues, with the bulge exhibiting a yellow-white color. There are no prominent dust lanes or spiral arm structures visible in the image, and the galaxy appears relatively undisturbed, showing no strong signs of recent major merging events or tidal interactions. There may be some low-level star formation occurring within the galaxy, suggested by the presence of some bluer hues, but the dominant color indicates the star formation is not extremely vigorous.
