This galaxy appears to be a relatively smooth, elliptical system. The light profile suggests a concentrated central bulge region with a gradual decline in luminosity towards the outer regions. The shape is elongated, exhibiting an aspect ratio that could be described as cigar-shaped. While it has a smooth morphology, there is a slight irregularity in the disk indicating minor disturbances. The color index suggests a population dominated by older stars, particularly in the bulge, which displays a more yellowish hue. A small amount of blue light indicates ongoing star formation. There is no evidence of a major merger or strong tidal interactions.
