The galaxy presents as a moderately luminous object with an elliptical morphology. The light distribution appears relatively smooth. There is a slight elongation, and a cigar-like shape. The central region exhibits a higher concentration of light, gradually decreasing towards the outer edges. Color gradients across the galaxy are subtle, with the core appearing slightly redder than the outskirts, suggesting potentially older stellar populations in the center. There's no visual evidence of spiral arms or strong dust lanes. The galaxy appears relatively isolated, without any obvious signs of recent major mergers or tidal interactions. There are no obvious features in the image that would suggest a high rate of on-going star formation.
