The galaxy appears to be an elliptical galaxy, characterized by its smooth, spheroidal morphology and lack of prominent spiral arms or a distinct disk structure. The galaxy exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. The color distribution appears to be relatively uniform, with a slight yellowish hue, suggesting a population of older stars and a lack of significant ongoing star formation. There is no evidence of any major mergers or tidal disturbances in the immediate vicinity of the galaxy, indicating that it has likely evolved in relative isolation. It seems to be fairly round, as opposed to a cigar shape.
