The galaxy appears to be an elliptical type, exhibiting a smooth, generally round morphology. A slight elongation is present, suggesting it is not perfectly spherical. The color profile displays a central bulge that is predominantly yellow-orange, indicative of an older stellar population. Moving outwards from the core, a subtle transition towards a redder hue is observed. A faint feature exists extending vertically, appearing separate from the galaxy and exhibiting a redder profile. The overall structure appears undisturbed, lacking the distinct features associated with recent major mergers, yet may be undergoing minor gravitational interactions. Star formation appears to be relatively quiescent based on the color indices.
