The galaxy presents a generally elliptical morphology with a bright, concentrated central bulge. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or distinct features. Some asymmetry is present in the outer regions. The color gradient shifts from yellowish-white at the core, possibly indicating older stellar populations, to bluish hues in the outer regions, suggestive of ongoing or recent star formation, though this is faint. Overall, the galaxy exhibits an intermediate redshift. The shape can be quantified to be elliptical. The estimated physical size is roughly 5 kpc in radius. The light from the galaxy is dominated by redder wavelengths with increasing signal in green and blue wavelengths. Evidence of past or minor mergers cannot be excluded.