The galaxy presents a generally smooth appearance, exhibiting a concentrated central bulge. The morphology suggests a spheroidal or elliptical classification, with a moderate elongation visible in the image. The color gradient indicates an older stellar population, with a yellowish hue dominating the core, and slightly bluer colors towards the outer regions. There's little evidence of prominent spiral arms or significant dust lanes. No distinct features are visible to suggest any active merging events. The galaxy appears relatively isolated and undisturbed within the observed field.
