The galaxy presents a somewhat elongated, cigar-shaped morphology. Its overall structure appears relatively smooth, exhibiting a diffuse, blended light distribution without any clear spiral arm structures or prominent star-forming regions immediately visible. The color gradient suggests a central concentration of older stellar populations, appearing slightly redder, gradually transitioning to bluer hues towards the outer regions. This may indicate ongoing star formation, albeit at a low rate, or a difference in the age and composition of the stellar populations at different radii within the galaxy. There is a subtle hint of a possible minor disturbance or tidal feature in the galaxy's shape, perhaps indicative of a past or ongoing interaction with a smaller companion, though no clear merging event is evident.
