The galaxy presents a generally smooth, elliptical morphology. It appears moderately rounded in shape, lacking any distinct spiral arm structures or a prominent central bar. There is a slight elongation. The light distribution is centrally concentrated, showing a gradual decrease in brightness from the core outwards. Color gradients are subtle, with a yellowish-orange hue suggesting a relatively older stellar population. There appears to be little to no evidence of active star formation regions within the galaxy itself based on the color. There might be a minor tidal disturbance or interaction occurring, or possibly a merger event, given the irregularities in the light distribution. Overall, the galaxy appears to be a relatively massive, evolved system likely composed of primarily older stars.
