The galaxy presents as a relatively compact, centrally concentrated object. Its overall structure appears smooth with no distinct spiral arm features or prominent dust lanes visible. The galaxy exhibits a nearly circular morphology, suggesting a minimal degree of ellipticity. The color profile seems to be relatively uniform throughout the galaxy, with a slightly higher concentration of redder hues towards the core region, potentially indicating an older stellar population or a higher dust content in the central regions. The outer regions of the galaxy appear to fade gradually into the background, suggesting a smooth transition in stellar density. There is a hint of a possible interaction or minor disturbance in the galaxy’s morphology. Upon closer examination, there seems to be some degree of tidal distortion or a faint plume extending from the main body. This could be indicative of a recent merger event or tidal interaction with a nearby companion galaxy.
