The galaxy appears as a relatively smooth, well-defined elliptical structure. Its morphology is largely spheroidal, with a high degree of roundness and no prominent disk features are clearly visible. There are no indications of major mergers or strong tidal disturbances in its immediate vicinity. A slightly brighter central bulge is present with luminosity decreasing steadily towards the outer edges of the galaxy, suggesting that the stellar population is composed of older, redder stars. The galaxy exhibits an overall even light distribution, implying a lack of significant internal structures or intense star-forming regions. Overall color indices suggest that the stellar population is composed of older stars. There is no indication of very active star formation in the galaxy, as the presence of strong H-alpha emissions are not seen in this image.
