The galaxy presents with a diffuse morphology, appearing neither purely elliptical nor fully spiral. A central bulge, brighter in appearance, is discernable, surrounded by a fainter, more extended halo. The shape of the galaxy leans toward a somewhat flattened spheroid, not quite circular but also not highly elongated.

There are indications of disturbance in the galaxy's structure, possibly due to a past or ongoing interaction. Faint tidal features or irregularities can be observed around the galaxy's periphery. The color profile suggests a mix of stellar populations; the central region exhibits a bluer hue indicative of younger, hotter stars, while the outer regions appear redder, potentially hosting older, cooler stellar populations. Areas of dust extinction or star formation are not clearly prominent within the visible structure of this galaxy.
