The galaxy appears to be a relatively compact object, exhibiting a generally elliptical morphology. A bright, concentrated central bulge is apparent, surrounded by a more diffuse halo. The color gradient suggests a blue-white core, potentially indicative of ongoing star formation within the bulge. Fainter, reddish hues appear in the outer regions, hinting at an older stellar population and/or dust extinction in the periphery. There is very slight asymmetry present. No distinct spiral arms or bar structures are discernible. The galaxy exhibits only minor morphological disturbances, suggesting it is not currently undergoing major merger activity, although there is an indication of some form of minor interaction. Overall, the galaxy appears to be a mid-sized system, possibly of an intermediate Hubble type between elliptical and early spiral, with some features indicative of ongoing star formation in the central region.
