The galaxy appears as a centrally concentrated, luminous object with an overall smooth morphology. It exhibits a generally elliptical shape, appearing more rounded than elongated. There is some evidence of a possible secondary concentration of light in the upper left quadrant, suggesting a minor disturbance in the galaxy's structure, possibly indicative of an ongoing or past minor merger event. The galaxy is primarily yellow and red in hue, indicating a population of older stars and a relatively low rate of recent star formation. There are faint, diffuse extensions of light surrounding the central core, but no readily discernible spiral arm structure or prominent dust lanes are visible. The galaxy's light distribution appears relatively even across its extent, suggesting that it is not a highly active star-forming system.
