The galaxy appears to be a relatively compact, elliptical or lenticular type system. The light distribution is generally smooth, with a central concentration of luminosity that gradually decreases towards the outer regions. There is no obvious spiral arm structure or prominent dust lane visible in the image, which further supports this classification. The galaxy displays a subtle color gradient, with a more yellowish hue towards the center, suggesting a population of older stars in the bulge. The outer regions are slightly bluer, which could indicate the presence of younger stars, although the overall star formation rate appears low. The galaxy exhibits a round to slightly elongated shape, showing no signs of major mergers or significant tidal disturbances. Based on its characteristics, it is likely a galaxy with a considerable mass and a low specific star formation rate.
