This galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated luminosity profile. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy appears elongated, with a moderate ellipticity, and is nearly edge-on from our vantage point.

The core of the galaxy shows a bright, yellowish-white hue, suggesting an older stellar population. This central concentration graduates into a surrounding halo that diffuses outwards, demonstrating a lower surface brightness. The outer regions are subtly tinged with bluish color, which may indicate the presence of some younger, hotter stars at the periphery, but this appears subdued. There is no obvious indication of recent major merger activity or tidal tails, though subtle disturbances cannot be ruled out at this resolution. Overall, this galaxy seems to represent a fairly evolved system with a significant fraction of older stars and low levels of ongoing star formation.
