The galaxy presents as a smooth, elliptical morphology. Its shape is elongated, with a high degree of oblateness, appearing cigar-shaped. The central region displays a concentration of light with a yellow-orange hue, suggesting an older stellar population. The outer regions exhibit a gradual decrease in luminosity, with a subtle transition towards a bluer color, possibly indicating the presence of some younger stars but still dominated by older stars. The galaxy lacks any obvious spiral arms or distinct dust lanes. There is no evidence of any significant ongoing merger activity or major disturbances in its overall structure. It appears to be a relatively isolated system, exhibiting no strong tidal interactions with nearby galaxies.
