The galaxy presents an overall smooth morphology with a generally elliptical shape. The central region exhibits a concentrated, luminous core appearing as a bright, yellowish-orange hue, indicative of an older stellar population or dust obscuration. Moving outward from the core, the galaxy gradually fades, displaying a less intense, more diffuse distribution of light. There is a subtle suggestion of a flattened structure, but no distinct spiral arms or prominent features are visible. The galaxy exhibits no strong signs of active merging or tidal disturbances, presenting a seemingly relaxed structure. Color variations across the galaxy are subtle, with a gradual shift toward bluer hues in the outer regions. 
