The galaxy presents a generally elliptical morphology with an inclination that suggests it is viewed at a moderate angle. A prominent central bulge is observed, exhibiting a smooth, concentrated light distribution that fades gradually towards the outer regions. There is evidence of some disk-like structure. Some asymmetry is present; a possible sign of gravitational interactions. A region of bluer light is observed within the galaxy, possibly indicative of younger stellar populations and ongoing star formation within localized regions. The overall color of the galaxy is skewed towards the redder part of the spectrum, indicating an older stellar population and lower levels of recent star formation compared to a bluer spiral galaxy. The galaxy exhibits a relatively smooth profile, with limited evidence of strong spiral arms or prominent dust lanes.
