The galaxy appears to be relatively compact. It displays a central bulge region that exhibits a smoother texture and a reddish hue, indicative of an older stellar population. The galaxy's outer regions present a bluer color, suggesting the presence of younger, hotter stars. There are some indications of faint, extended structures or tidal features that could point to possible interactions with nearby galaxies. Overall, the galaxy shows a complex morphology, possibly a product of past or ongoing gravitational interactions. Further spectroscopic analysis may be beneficial to identify the nature of the galaxy.
