The galaxy presents an overall smooth appearance, with a concentrated central bulge that appears somewhat yellowish, suggesting an older stellar population in the core. There may be a faint disk structure or arm feature extending from the central region, seen more clearly as less concentrated emission. These regions have patches of redder emission. The galaxy exhibits an elliptical-like morphology in terms of the bulge, appearing rather rounded. There is a minor visual disturbance, possibly indicative of an interaction or minor merger event affecting the disk. The galaxy appears relatively compact, with a defined boundary.
