The galaxy presents as a concentrated central bulge surrounded by a less defined, more diffuse disk. The galaxy exhibits an overall roundish morphology, though it is not perfectly circular. The color profile suggests a mixed stellar population; the central bulge appears yellower, potentially indicating older, redder stars, while the disk shows some bluer tones, hinting at the presence of younger, hotter stars and ongoing star formation. No significant signs of a major ongoing merger or disruption are immediately visible. There appears to be some minor disturbance in the form of asymmetry.
