The galaxy presents an elongated, roughly elliptical morphology. The light profile appears smooth, with no distinct spiral arm structures or prominent dust lanes visible. There is a concentration of light toward the central region, suggestive of a bulge component. The color is generally yellowish-white, with a slight gradient towards bluer hues at the outer edges. This color distribution indicates a mix of stellar populations, possibly with relatively older stars dominating the central region and younger, hotter stars present in the outer regions. The smoothness of the light distribution suggests that it may be an early-type spiral or elliptical galaxy, likely with a significant population of older stars, and with recent evidence of some star formation. No obvious signs of tidal disturbances or ongoing mergers are immediately apparent.
