The galaxy presents as a moderately luminous object at a redshift of approximately 0.12. It appears to be a relatively smooth, early-type galaxy, likely elliptical or lenticular, exhibiting minimal discernible substructure. The light distribution is concentrated towards the center, with a gradual decline in surface brightness moving outwards. Its overall shape appears mostly round, with only a small deviation from perfect circularity, suggesting a low degree of inclination relative to our line of sight. No prominent dust lanes, spiral arms, or other features indicative of ongoing star formation are immediately apparent in the available imagery. This observation suggests a galaxy where star formation activity is either quiescent or significantly reduced. There is no visible evidence of any recent or ongoing major merger events, tidal tails, or other disruptive features. The light is dominated by longer wavelengths, with a gradual shift towards redder colors, this could be associated with an older stellar population.
