The galaxy presents with a generally elliptical morphology, exhibiting a central, relatively smooth light distribution that transitions into fainter, more diffuse outskirts. The core region displays a bluish hue, potentially indicative of a younger stellar population or active star formation. A noticeable, more elongated component extends outward, with a shift towards yellower color, hinting at an older stellar population.

There appear to be subtle irregularities in the galaxy's structure, possibly a minor disturbance in its morphology. Alternatively, it could be indicative of recent or ongoing interactions with another galaxy, though no clear merging companion is immediately apparent in the surrounding field. The overall shape is largely rounded but shows hints of a distorted or asymmetric form.
