The galaxy presents a generally smooth morphology, with a notable lack of distinct spiral arms or a prominent central bulge. Its shape is elongated, suggesting a possible classification as an elliptical galaxy, although a highly inclined disk galaxy cannot be ruled out without further spectral analysis. The galaxy displays a colour gradient, appearing yellowish-white towards its center and gradually fading to a redder hue in the outer regions. There is little evidence of ongoing major mergers or tidal disturbances. A slight asymmetry in the outer regions hints at potential minor interactions, but the overall structure is predominantly undisturbed. The galaxy's relatively compact size and smooth appearance suggest a potential evolved stellar population. Star formation appears to be minimal.
