The galaxy presents as a relatively smooth, elliptical-like structure, with a centrally concentrated luminosity profile.  The light distribution exhibits a moderate degree of ellipticity but is largely rounded in shape.  There is little evidence of spiral arms or a significant disk component.  The galaxy appears fairly isolated, with no obvious signs of major tidal disturbances or ongoing mergers with other galaxies, though a slight asymmetry may suggest a minor past interaction. The overall color is consistent with a population of older stars, showing a redder hue, implying a relatively low rate of ongoing star formation. The galaxy is of intermediate size when compared to other galaxies.
