This galaxy appears to be an elliptical type galaxy, exhibiting a generally smooth and featureless morphology. There is some elongation, suggesting it is not perfectly spherical, leaning towards a more lenticular shape. The light is centrally concentrated with a bright core, gradually fading towards the edges. The color profile indicates a dominance of older stellar populations, primarily emitting in the redder wavelengths of the spectrum, with some contribution from green wavelengths as well. This is typical of galaxies with low star formation rates. There is no evident spiral arm structure or significant dust lanes. No signs of major mergers or significant tidal disturbances are obvious. Overall, the galaxy presents a well-defined, relaxed structure.
