The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with a concentrated central bulge. It presents a slightly elongated shape with an approximate ellipticity of 0.26, inclined at an angle of about 116 degrees. The galaxy's color profile shows a gradual shift from redder hues in the central region to bluer tones in the outer areas. The size suggests it is a relatively large galaxy, with a diameter possibly around 9 kpc. There is no obvious evidence of strong spiral arm structures or significant disturbances suggestive of ongoing mergers. The galaxy's overall appearance indicates a mature stellar population, although some level of star formation is likely still present.
