The galaxy presents as a faint, elongated structure with a distinct central bulge. It exhibits a generally smooth morphology, with minimal discernible spiral arm structure or prominent star-forming regions. The color profile suggests a population of older stars, possibly indicating a relatively quiescent state of star formation. The galaxy's elongated shape suggests that it could be an elliptical galaxy or a spiral galaxy viewed at an oblique angle. There may be some subtle disturbances indicative of a possible past or ongoing minor interaction. The galaxy appears to be an isolated entity within its immediate field, showing no signs of a major ongoing merger. 
