The galaxy appears as a moderately bright, relatively compact object. It exhibits a smooth, elliptical morphology with no readily apparent spiral arm structure. The galaxy displays a bright central bulge which fades into a less luminous halo. The color profile shows a dominance of redder hues, particularly in the central regions, transitioning toward bluer colors in the outer edges of the galaxy, suggesting a population of older stars centrally concentrated and younger stars in the outer regions. There is a slight flattening observed, indicating it is not perfectly spherical. There are no signs of tidal tails or other indications of a major recent merger. The galaxy is a relatively isolated system, with no nearby galaxies suggesting any current gravitational interaction.
