The galaxy appears to be an elliptical type, exhibiting a smooth, spheroidal morphology. Its light profile suggests a high degree of central concentration, with a bright core that gradually fades into the outer regions. There is no evidence of distinct spiral arms or a prominent disk structure. The color is generally redder, suggesting an older stellar population with relatively low ongoing star formation activity. No significant tidal features or signs of recent major mergers are apparent, indicating a dynamically relaxed state. Subtle color variations exist within the galaxy, but they are not indicative of substantial dust lanes or localized regions of intense star formation. The galaxy appears relatively isolated, with no obvious companion galaxies in close proximity that could be influencing its morphology or evolution.
