The galaxy presents a roughly elliptical morphology, although its structure appears somewhat complex upon closer inspection. The central region displays a bright, concentrated core, which transitions into a more diffuse halo. There is evidence of some structural disturbance, possibly indicative of a recent minor merger or tidal interaction. The disturbance is not major but can be observed on one side.

The color distribution suggests variations in stellar populations or dust content throughout the galaxy. The central core exhibits a bluer hue, potentially signifying a younger stellar population or lower dust obscuration compared to the outer regions. The outer regions are characterized by a redder color, which might indicate the presence of older stars or higher dust concentration.

The overall luminosity of the galaxy seems moderate. While the central core is quite luminous, the halo is less pronounced.
