The galaxy presents as a flattened elliptical form, its overall shape approximating a spheroid viewed at an angle. The central region exhibits a high surface brightness, suggesting a concentrated stellar population. The luminosity decreases gradually towards the outer edges. The color profile shows a predominantly yellowish-white hue in the core, shifting towards a bluer tint in the surrounding regions. This may indicate the presence of younger stellar populations in the outer areas. There is no clear evidence of spiral arm structures or a prominent dust lane from this vantage point. The galaxy appears relatively isolated, showing no signs of major tidal disruption or interaction with other galaxies. A minor perturbation might be present at one edge of the galaxy but it is difficult to say for sure.