The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a higher concentration of light, appearing more yellow, suggesting a higher population of older stars. Moving outwards from the core, the light gradually fades, with a reddish hue suggesting a presence of dust. The overall shape indicates a spheroid, and it is elongated, appearing cigar-shaped. There are no distinct spiral arms or obvious signs of recent major merger activity. Subtle disturbances or minor interactions might be occurring, but these are not clearly defined in the image. The galaxy's estimated size implies it is a substantial system. Star formation is present, but is not dominant.
