The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth morphology. It is elongated with a somewhat cigar-shaped appearance. A central bulge is evident with a smooth transition to the outer regions. There is no apparent spiral arm structure or dust lane visible in the image. The color profile suggests a mix of stellar populations, with the central bulge potentially exhibiting a more red-shifted hue, indicative of older stars, while the outer regions may be a bit bluer suggesting the presence of younger stars, though this is not clear given the quality of the image. Faint extensions or tidal features may be present but are difficult to discern. The galaxy does not appear to be undergoing a major merger, but might be experiencing a minor disturbance.