The galaxy presents as a relatively smooth, elliptical structure, with a high degree of central concentration. There is an apparent lack of prominent spiral arms or a well-defined disk. The color profile suggests an older stellar population, with a yellowish hue dominating the central region, indicating a paucity of ongoing star formation. The morphology appears largely undisturbed, with no strong evidence of recent major mergers or tidal interactions. The object exhibits a slight elongation, deviating marginally from a perfectly circular shape. There is no apparent dust lane or significant blue star forming regions. Light is distributed relatively evenly, and fades gradually towards the periphery.
