The galaxy presents a predominantly smooth morphology, suggesting a possible elliptical or lenticular classification. The central region displays a high degree of luminosity with a yellow-white hue, potentially indicative of an older stellar population. The overall shape appears to be somewhat rounded, although not perfectly spherical. There appears to be some disturbance in the light distribution, possibly due to minor interactions or internal dynamics. The redder color on the periphery may indicate regions of older, dustier stellar populations or background sources. The limited resolution restricts detailed analysis of any spiral arm structure or star-forming regions. Overall, the galaxy appears to be a moderately massive, relatively quiescent system at a redshift of approximately 0.13.
