The galaxy presents a morphology indicative of an elliptical or lenticular type. The light distribution appears smooth, with no readily discernible spiral arms or prominent dust lanes. It exhibits a generally elongated shape, though not markedly so. The core region shows a relatively high surface brightness. There is some irregularity in the outskirts of the galaxy, which might indicate a possible past or ongoing interaction, or simply an artifact of the limited resolution. The color profile appears to be redder, suggestive of an older stellar population with reduced ongoing star formation. Based on the overall smoothness and color, this is likely an evolved galaxy.
