The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. It exhibits a somewhat elliptical shape, leaning more towards a rounded appearance than a highly elongated one. The central region is characterized by a bright, yellowish-white core that gradually fades into a fainter, bluer outer region. There's no clear evidence of spiral arm structure or prominent dust lanes visible. The overall structure suggests the galaxy may be an early-type spiral or lenticular galaxy, with a significant spheroidal component. Slight disturbances are possibly visible in the surrounding region, but appear to be negligible, with no signs of a major ongoing merger or significant tidal features. The color gradient, from yellow-white at the center to bluer at the edges, might suggest a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars more prevalent in the outskirts.
