The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. The light distribution is concentrated towards the center, with a diffuse halo fading outwards. The color profile suggests a dominant population of older stars, indicated by the yellowish hue in the core. There is a slight elongation visible, suggesting it is not perfectly spherical. No obvious spiral arm structures or significant dust lanes are discernible in this image. There are hints of a very faint, bluish outer envelope, possibly indicative of a small population of younger stars or recent minor merger activity, though it is not distinct. There is no obvious evidence of strong tidal disturbances or ongoing major mergers.
