The galaxy presents as a relatively smooth, elliptical-like structure, with a high concentration of light towards its center. The morphology appears to be dominated by a bulge component with a radial falloff in intensity. The color profile suggests a population of older stars throughout the galaxy, exhibiting a slightly redder hue overall, which may signify a relatively low star formation rate. The galaxy exhibits an elongated shape, possibly indicating it is more of an in between round and cigar shaped galaxy. There are no visible spiral arm structures or significant dust lanes, supporting the smooth morphology classification. There is no evidence of ongoing major mergers or tidal disturbances in this image.
