The galaxy presents as a slightly elongated spheroid, with a central bulge that appears yellowish-white, suggesting an older stellar population. This is surrounded by a bluer, more diffuse halo. There may be some evidence of a faint, indistinct disk structure, but it's difficult to resolve any spiral arms. Overall, the galaxy appears relatively smooth. There are some minor disturbances present, and these might be signs of a minor merger or tidal interaction. The galaxy demonstrates signs of star formation, but it appears to be occurring at a moderate rate.
