The galaxy presents an elongated, cigar-shaped morphology, suggesting it may be an elliptical galaxy viewed at an angle or a spiral galaxy seen edge-on. A smooth, centrally concentrated bulge dominates the galaxy's luminosity. There's a gradual color gradient moving outward from the central bulge, going from a yellow hue towards a redder tone. The absence of distinctly resolved star-forming regions and a relatively smooth light profile suggest a lack of significant ongoing star formation, and that the galaxy primarily hosts an older stellar population. There is no clear evidence of any tidal features or significant signs of interaction or merging activity. The galaxy appears relatively undisturbed.
