The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, with a radial decrease in intensity. There is no prominent disk structure apparent in the image. The galaxy appears to be of moderate size and exhibits a yellowish-red hue, suggesting a population of older stars. There is a slight asymmetry in its shape, possibly indicative of a minor gravitational disturbance or interaction, although there is no clear evidence of a major merger event. The galaxy does not display strong signs of ongoing star formation.
