The galaxy presents as a moderately bright object with a somewhat elliptical morphology, exhibiting a significant central bulge. The color profile suggests an older stellar population, with a yellowish hue dominating the central regions. Fainter, bluer regions can be discerned peripherally, hinting at ongoing, though limited, star formation within the galaxy's disk. There are hints of slight disturbances or tidal features. The overall structure appears relatively smooth, with a notable absence of well-defined spiral arms. The galaxy's apparent intermediate roundness suggests that we observe it from an intermediate angle to its rotational axis. There is also a lack of strong indicators of a major ongoing merger event.
