The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light distribution. There is a noticeable absence of spiral arm structure or prominent dust lanes. The core of the galaxy presents a yellowish hue, which might be indicative of an older stellar population. The galaxy's light profile gradually fades towards the outer edges, suggesting a diffuse halo surrounding the brighter central region. A faint, slightly elongated structure hints at a possible disk component or tidal disturbance, although the overall morphology is dominated by its smooth, spheroidal shape. There is a minor hint of blue light in the outer fringes of the galaxy, perhaps showing a small amount of recent star formation. The object appears relatively isolated, with no obvious signs of ongoing major mergers or strong gravitational interactions with other nearby galaxies.
